The SUDARE SN survey was performed using the VLT Survey Telescope (VST) equipped with the OmegaCAM camera, that started regular operations in October 2011 at ESO Paranal (Chile). The VST has a primary mirror of 2.6m and a f/5.5 modified Ritchey-Chretien optical layout that is designed to deliver a large, uniform focal plane. SUDARE is a four-year programme and this paper is devoted to analysing the first two observing seasons for VOICE-CDFS and one season for COSMOS. We are currently completing the monitoring of both fields for the two subsequent seasons. (1 data file).